The Possible Signs of Hydrogen and Helium Accretion from Interstellar Medium on the Atmospheres of F-K Giants in the Local Region of the Galaxy |
Yushchenko, Alexander
(Astrocamp Contents Research Institute)
Kim, Seunghyun (Astrocamp Contents Research Institute) Jeong, Yeuncheol (History Department, Sejong University) Demessinova, Aizat (Physico-Technical Department, Al Farabi Kazakh National University) Yushchenko, Volodymyr (Main Astronomical Observatory of National Academy of Sciences of Ukraine) Doikov, Dmytry (Department of Natural and Technical Sciences, Odessa National Maritime University) Gopka, Vira (Astronomical Observatory, Odessa National University) Jeong, Kyung Sook (DaeYang Humanity College, Sejong University) Rittipruk, Pakakaew (National Astronomical Research Institute of Thailand) |
1 | Asplund M, Amarsi AM, Grevesse N, The chemical make-up of the Sun: a 2020 vision, Astron. Astrophys. in press (2021). https://arxiv.org/pdf/2105.01661 |
2 | Bohm-Vitense E, The puzzle of the metallic line stars, Publ. Astron. Soc. Pac. 118, 419-435 (2006). https://doi.org/10.1086/499385 DOI |
3 | Burbidge EM, Burbidge GR, Fowler WA, Hoyle F, Synthesis of the elements in stars, Rev. Mod. Phys. 29, 547-650 (1957). https://doi.org/10.1103/RevModPhys.29.547 DOI |
4 | Castelli F, Kurucz R, New grids of ATLAS9 model atmospheres, in IAU Symposium 210, Uppsala, Sweden, 17-21 Jun 2002. |
5 | Cowan JJ, Sneden C, Lawler JE, Aprahamian A, Wiescher M, et al., Origin of the heaviest elements: the rapid neutron-capture process, Rev. Mod. Phys. 93, 015002 (2021). https://doi.org/10.1103/RevModPhys.93.015002 DOI |
6 | Cowley CR, Bord DJ, The CP stars, an overview: then and now, IAU Symp. 224, 265-281 (2004). https://doi.org/10.1017/S174392130400465X DOI |
7 | Drobyshevski EM, Peculiar A-stars and planetary systems, Astrophys. Space Sci. 35, 403-408 (1975). https://doi.org/10.1007/BF00637006 DOI |
8 | Erspamer D, North P, Automated spectroscopic abundances of A and F-type stars using echelle spectrographs. II. Abundances of 140 A-F stars from ELODIE, Astron. Astrophys. 398, 1121-1135 (2003). https://doi.org/10.1051/0004-6361:20021711 DOI |
9 | Fowler WA, Burbidge EM, Burbidge GR, Hoyle F, The synthesis and destruction of elements in peculiar stars of types A and B, Astrophys. J. 142, 423-450 (1965). https://doi.org/10.1086/148309 DOI |
10 | Greenstein JL, Analysis of the metallic-line stars. II. Astrophys. J. 109, 121-138 (1949). https://doi.org/10.1086/145112 DOI |
11 | Grevesse N, Asplund M, Sauval AJ, Scott P, The chemical composition of the Sun, Astrophys. Space Sci. 328, 179-183 (2010). https://doi.org/10.1007/s10509-010-0288-z DOI |
12 | Havnes O, Conti PS, Magnetic accretion processes in peculiar A stars, Astron. Astrophys. 14, 1-11 (1971). |
13 | Jeong Y, Yushchenko A, Gopka V, Yushchenko V, Rittipruk P, et al., The barium star HD204075: iron abundance and the absence of evidence for accretion, J. Astron. Space Sci. 36, 105-113 (2019). https://doi.org/10.5140/JASS.2019.36.3.105 DOI |
14 | Havnes O, Magnetic stars as generators of cosmic rays, Astron. Astrophys. 13, 52-57 (1971). |
15 | Jeong Y, Yushchenko AV, Doikov DN, Gopka VF, Yushchenko VO, Chemical composition of RR Lyn - an eclipsing binary system with Am and λ Boo type components, J. Astron. Space Sci. 34, 75-82 (2017). https://doi.org/10.5140/JASS.2017.34.2.75 DOI |
16 | Kang YW, Yushchenko AV, Hong K, Guinan EF, Gopka VF, Signs of accretion in the abundance patterns of the components of the RS CVn-type eclipsing binary star LX Persei, Astron. J. 145, 167 (2013). https://doi.org/10.1088/0004-6256/145/6/167 DOI |
17 | Kim C, Yushchenko AV, Kim SL, Jeon YB, Kim CH, Chemical composition and photometry of BE Lyncis, Publ. Astron. Soc. Pac. 124, 401-410 (2012). https://doi.org/10.1086/665943 DOI |
18 | Luck RE, Abundances in the local region. I. G and K giants, Astron. J. 150, 88 (2015). https://doi.org/10.1088/0004-6256/150/3/88 DOI |
19 | Michaud G, Diffusion processes in peculiar A stars, Astrophys. J. 160, 641 (1970). https://doi.org/10.1086/150459 DOI |
20 | Niemczura E, Morel T, Aerts C, Abundance analysis of prime B-type targets for steroseismology. II. B6-B9.5 stars in the field of view of the CoRoT satellite, Astron. Astrophys. 506, 213-233 (2009). https://doi.org/10.1051/0004-6361/200911931 DOI |
21 | Neiner C, Wade GA, Sikora J, Discovery of a magnetic field in the δ Scuti F2m star ρ Pup, Mon. Not. R. Astron. Soc. Lett. 468, L46-L49 (2016). https://doi.org/10.1093/mnrasl/slx023 DOI |
22 | North P, The rotation of AP stars, Astron. Astrophys. 141, 328-340 (1984). |
23 | Proffitt CR, Michaud G, Abundance anomalies in A and B stars and the accretion of nuclear-processed material from supernovae and evolved giants. Astrophys. J. 345, 998-1007 (1989). https://doi.org/10.1086/167969 DOI |
24 | Tanaka SJ, Chiaki G, Tominaga N, Susa H, Blocking metal accretion onto population III stars by stellar wind, Astrophys. J. 844, 137 (2017). https://doi.org/10.3847/1538-4357/aa7e2c DOI |
25 | Venn KA, Lambert DL, Could the ultra-metal-poor stars be chemically peculiar and not related to the first stars, Astrophys. J. 677, 572 (2008). https://doi.org/10.1086/529069 DOI |
26 | Wallerstein G, Iben Jr. I, Parker P, Boesgaard AN, Hale GM, et al., Synthesis of the elements in stars: forty years of progress, Rev. Mod. Phys. 69, 995-1084 (1997) https://doi.org/10.1103/RevModPhys.69.995 DOI |
27 | Yushchenko AV, Jeong Y, Gopka VF, Vasileva SV, Andrievsky SM, et al., Chemical composition of RM_1-390-large magellanic cloud red supergiant, J. Astron. Space Sci. 34, 199-205 (2017a). https://doi.org/10.5140/JASS.2017.34.3.199 DOI |
28 | Yushchenko AV, Gopka VF, Kang YW, Kim C, Lee BC, et al., The chemical composition of ρ puppis and the signs of accretion in the atmospheres of B-F-type stars, Astron. J. 149, 59 (2015). https://doi.org/10.1088/0004-6256/149/2/59 DOI |
29 | Yushchenko AV, Gopka VF, Shavrina AV, Yushchenko VA, Vasileva SV, et al., Peculiarities of the abundance of chemical elements in the atmosphere of PMMR23-red supergiant in the small magellanic cloud due to interstellar gas accretion, Kinemat. Phys. Celest. Bodies. 33, 199-216 (2017b). https://doi.org/10.3103/S0884591317050075 DOI |
30 | Yushchenko AV, Kim C, Jeong Y, Dmytry DN, Volodymyr YA, et al., The chemical composition of V1719 Cyg: δ Scuti type star without the accretion of interstellar matter, J. Astron. Space Sci. 37, 157-163 (2020). https://doi.org/10.5140/JASS.2020.37.3.157 DOI |
31 | Kang YW, Yushchenko A, Hong K, Kim S, Yushchenko V, Chemical composition of the components of eclipsing binary star ZZ Bootis, Astron. J. 144, 35 (2012). https://doi.org/10.1088/0004-6256/144/2/35 DOI |
32 | Cowley CR, An examination of the planetesimal impact hypothesis of the formation of CP stars, Astrophys. Space Sci. 51, 349-362 (1977). https://doi.org/10.1007/BF00644158 DOI |
33 | Venn KA, Lambert DL, The chemical composition of three lambda Bootis stars, Astrophys. J. 363, 234-244 (1990). https://doi.org/10.1086/169334 DOI |
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